Interaction of the WAT Source in A3395 with the Intracluster Medium

Details Interaction of the WAT Source in A3395 with the Intracluster Medium Interaction of the WAT Source in A3395 with the Intracluster Medium

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011japa...32..493l&link_type=abstract

Journal of Astrophysics and Astronomy, Vol. 32, p. 493-494

Astronomy and Astrophysics

Astrophysics

Galaxies: Clusters: General, Galaxies: Clusters: Individual: (A3395), Galaxies: Clusters: Intracluster Medium, X-Rays: Galaxies: Clusters, Radio Continuum: Galaxies

Scientific paper

Using X-ray observations from Chandra and XMM-Newton and radio observations from the Australia Telescope Compact Array (ATCA), we have examined the merging environment of the bimodal cluster Abell 3395. From X-ray data we have produced thermodynamic maps of the cluster. The Wide Angle Tail (WAT) galaxy seen in the radio is slightly offset from the X-ray emission peak of the southern part of the cluster. The unsharp masked Chandra image of the cluster does not show any deficit in the X-ray flux near the location of the source possibly because the thermal plasma has leaked into the cavities.

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